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Fig. 1

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Azimuthally averaged profiles of the disk gas and dust surface density as well as the midplane temperature. The disk is evolved adiabat-ically with a constant α = 10−3 to show the pseudo-equilibrium of the initial configuration (solid lines) after 50 kyr of evolution (dashed lines). The gray band shows the water snow region. The dotted line marks Rend, outside of which an exponential taper is applied.

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